This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 04 48.93 +62 24 24.5 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1895937,2461140.6528,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1895937 20260410.1528 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 10.1528 2461140.6528 8.82 03:08:10.83 +59:02:12.7
139.73596 0.70084 galactic Cas Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 varaible 462749298419060864 | 03:08:10.57 +59:02:09.1 (Gaia DR3) | LPV (Gaia DR3) | 2022yCat.1358....0G | Gaia3var=VARIABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: M7 1947AnDea...5....1L DO 26691
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 08 10.83 +59 02 12.7 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 462749298419060864,2461140.6528,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 462749298419060864 20260410.1528 8.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 54 19.68 +59 29 18.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1936142,2461140.6528,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1936142 20260410.1528 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 57 11.63 +57 30 30.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J025711.21+573025.5,2461140.6528,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J025711.21+573025.5 20260410.1528 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 48 50.66 +64 11 50.7 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024850.01+641152.3,2461140.6528,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J024850.01+641152.3 20260410.1528 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 05 29.70 +62 47 01.2 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J030529.53+624701.2,2461140.6528,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J030529.53+624701.2 20260410.1528 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 58 19.49 +62 25 47.0 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1891924,2461140.6528,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1891924 20260410.1528 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 56 49.69 +58 14 29.2 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J044.2060+58.2406,2461140.6528,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J044.2060+58.2406 20260410.1528 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2041302,2461140.6528,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2041302 20260410.1528 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0338100+594043,2461140.6528,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0338100+594043 20260410.1528 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 08 46.31 +57 48 41.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J047.1932+57.8106,2461140.6528,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J047.1932+57.8106 20260410.1528 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J033009.09+644631.9,2461140.6528,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J033009.09+644631.9 20260410.1528 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GN Cam,2461140.6528,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GN Cam 20260410.1528 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 53 45.32 +58 57 49.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZALD J02534456+5857442,2461140.6528,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZALD J02534456+5857442 20260410.1528 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 04 57.04 +63 47 36.2 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J030456.65+634736.1,2461140.6528,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J030456.65+634736.1 20260410.1528 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 55 32.12 +58 16 20.3 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1936594,2461140.6528,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1936594 20260410.1528 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J031646.49+644506.3,2461140.6528,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J031646.49+644506.3 20260410.1528 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 10 30.40 +60 53 32.8 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J031030.06+605329.4,2461140.6528,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J031030.06+605329.4 20260410.1528 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2022346,2461140.6528,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2022346 20260410.1528 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 57 39.75 +58 12 52.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6528,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1528 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 00 52.89 +58 01 54.6 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J045.2194+58.0307,2461140.6528,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J045.2194+58.0307 20260410.1528 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0358411+640934,2461140.6528,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0358411+640934 20260410.1528 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 50 12.71 +60 56 24.0 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 464886779083679872,2461140.6528,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 464886779083679872 20260410.1528 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J032127.58+631536.3,2461140.6528,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J032127.58+631536.3 20260410.1528 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 00 45.53 +59 43 07.3 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0700 Cas,2461140.6528,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0700 Cas 20260410.1528 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J031913.92+584158.7,2461140.6528,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J031913.92+584158.7 20260410.1528 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 11 00.32 +58 25 10.7 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J031100.21+582507.3,2461140.6528,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J031100.21+582507.3 20260410.1528 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 12 53.33 +58 12 05.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J031253.14+581200.6,2461140.6528,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J031253.14+581200.6 20260410.1528 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J032633.00+613343.7,2461140.6528,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J032633.00+613343.7 20260410.1528 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J032408.33+600552.8,2461140.6528,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J032408.33+600552.8 20260410.1528 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1966431,2461140.6528,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1966431 20260410.1528 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 04 22.09 +61 25 44.0 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0506 Cas,2461140.6528,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0506 Cas 20260410.1528 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 56 24.52 +64 50 29.8 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J025623.98+645033.1,2461140.6528,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J025623.98+645033.1 20260410.1528 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NV Cam,2461140.6528,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NV Cam 20260410.1528 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0324152+575102,2461140.6528,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0324152+575102 20260410.1528 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 59 06.30 +57 48 33.6 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1939127,2461140.6528,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1939127 20260410.1528 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 51 21.12 +63 25 28.2 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CX Cas,2461140.6528,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CX Cas 20260410.1528 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 46 27.57 +63 40 33.0 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024627.15+634036.1,2461140.6528,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J024627.15+634036.1 20260410.1528 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 00 51.06 +58 56 33.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1940714,2461140.6528,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1940714 20260410.1528 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 48 00.11 +63 45 44.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024759.50+634541.0,2461140.6528,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J024759.50+634541.0 20260410.1528 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 00 48.04 +65 01 10.1 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J030047.67+650111.9,2461140.6528,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J030047.67+650111.9 20260410.1528 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 45 05.62 +65 01 20.9 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J024504.79+650123.4,2461140.6528,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J024504.79+650123.4 20260410.1528 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 58 15.24 +61 43 08.2 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J025814.83+614307.3,2461140.6528,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J025814.83+614307.3 20260410.1528 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 03 27.68 +60 07 46.4 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J030327.39+600744.1,2461140.6528,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J030327.39+600744.1 20260410.1528 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 03 06 39.86 +60 18 08.9 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J046.6659+60.3019,2461140.6528,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J046.6659+60.3019 20260410.1528 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 59 40.14 +62 33 39.3 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6528,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1528 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1528* 02 51 46.70 +59 27 47.0 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 464462784214490240,2461140.6528,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 464462784214490240 20260410.1528 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.58672519 21.01.2026 02:04:43.056 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461061.58672519 21.01.2026 02:04:43.056 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461140.65312123 10.04.2026 03:40:19.674 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18667
Objects passed selection criteria: 18566
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 13430.5
Average stars matched: 12349.5 (91.9512 %)
Memory usage VmPeak: 121860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:43:42 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.58672519 21.01.2026 02:04:43.056 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461061.58672519 21.01.2026 02:04:43.056 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461140.65312123 10.04.2026 03:40:19.674 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 138
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 42 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 134597
Objects passed selection criteria: 134175
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 95428.2
Average stars matched: 87505.2 (91.6974 %)
Memory usage VmPeak: 1896304 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:46:20 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
SExtractor catalog cache: saved Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461140.65251181
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
Saving wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits'
wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits exists and is non-empty
Saving wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits to local_wcs_cache/
'wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits'
wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits exists and is non-empty
Saving wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits to local_wcs_cache/
'wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits' -> 'local_wcs_cache/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:38.482 +62:00:06.69
Second-epoch image center 03:26:31.334 +61:58:41.29
Angular distance between the image centers 0.1061 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:38.482 +62:00:06.69
Second-epoch image center 03:26:29.420 +61:59:22.66
Angular distance between the image centers 0.1004 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:26:31.334 +61:58:41.29
Second-epoch second image center 03:26:29.420 +61:59:22.66
Angular distance between the image centers 0.01209 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.r9cLPMN85I
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.8jxMIJDleF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits &> /tmp/tmp.ZqrJRcugwJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits &> /tmp/tmp.BDy7Ldmywb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
Found non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
The reference image (wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat) found
'wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat' -> 'wcsmag.cat'
Read 21008 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.3293 to 69.9273 deg, Dec +55.1713 to +67.4989 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 31.3293 to 69.9273 deg, Dec 55.1713 to 67.4989 deg
Loaded 17842 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9611 out of 10566 total matches.
Matched with Tycho-2 10566 out of 21008 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.956154
a=0.000000 b=1.000000 c=22.956154
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
2.0 pix Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
2.7 pix fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
2.7 pix fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Limiting magnitude estimates:
15.4 mag. Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
15.4 mag. Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
14.5 mag. fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
14.5 mag. fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.r9cLPMN85I (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2066, passed=21008
Got 21008 stars (including 18916 good ones) from the SExtractor catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 21008 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 20553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 20554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 20553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8jxMIJDleF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2108, passed=21108
Got 21108 stars (including 18961 good ones) from the SExtractor catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 21108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 20649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 20649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 20650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZqrJRcugwJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1281, passed=12673
Got 12673 stars (including 11385 good ones) from the SExtractor catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 12673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 12362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 12365 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 12365 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits -region wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BDy7Ldmywb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Checking if the catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
WCS catalog name: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1321, passed=12717
Got 12717 stars (including 11390 good ones) from the SExtractor catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 12717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 12420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 12421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 12421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits -region wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits'
Saving fully-calibrated image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits'
Saving fully-calibrated image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits'
Preparing the HTML report for the field Cam-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out17276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12990.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33033_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 33033_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:37:09.48 +64:20:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15464_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 15464_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:56:47.84 +63:27:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17276_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 17276_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:48:50.56 +64:11:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 3.762 467753347639403776 042.20834848060 +64.19785504852 11.2922 9.9324 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12990_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 12990_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05502_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 05502_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07520_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 07520_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 19s
Prepared the HTML report for the field Cam-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:08:10.83 +59:02:12.7
02:54:19.68 +59:29:18.4
03:04:48.93 +62:24:24.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
SExtractor catalog cache: saved Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits exists and is non-empty
wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:38.482 +62:00:06.69
Second-epoch image center 03:26:31.334 +61:58:41.29
Angular distance between the image centers 0.1061 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:38.482 +62:00:06.69
Second-epoch image center 03:26:29.420 +61:59:22.66
Angular distance between the image centers 0.1004 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:26:31.334 +61:58:41.29
Second-epoch second image center 03:26:29.420 +61:59:22.66
Angular distance between the image centers 0.01209 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.aWwzWQOwG5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.2LSJM1GYY2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits &> /tmp/tmp.zz69RAhe4r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits &> /tmp/tmp.5GMTzDwFu0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
Found non-empty wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
The reference image (wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat) found
'wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat' -> 'wcsmag.cat'
Read 154615 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.2733 to 69.9681 deg, Dec +55.1712 to +67.5021 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 31.2733 to 69.9681 deg, Dec 55.1712 to 67.5021 deg
Loaded 17905 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 7837 out of 10776 total matches.
Matched with Tycho-2 10776 out of 154615 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815520
a=0.000000 b=1.000000 c=22.815520
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.59
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.59
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 121 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
1.9 pix Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
2.6 pix fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
2.6 pix fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Limiting magnitude estimates:
15.6 mag. Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
15.6 mag. Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
14.6 mag. fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
14.6 mag. fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.aWwzWQOwG5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=17751, passed=154592
Got 154592 stars (including 136576 good ones) from the SExtractor catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 154592 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 152245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 152245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 152245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2LSJM1GYY2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=17698, passed=153379
Got 153379 stars (including 135404 good ones) from the SExtractor catalog wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 153379 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 151084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 151083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 151084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zz69RAhe4r (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=8687, passed=73956
Got 73956 stars (including 65199 good ones) from the SExtractor catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 73956 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 72383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 72384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 72385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits -region wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5GMTzDwFu0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Checking if the catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
WCS catalog name: wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=10, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=8440, passed=73097
Got 73097 stars (including 64580 good ones) from the SExtractor catalog wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 73097 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 71763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 71767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 71765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits -region wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_Cam-08-Q2b1x1_2026-01-20_20-05-37_20.00sec_-15.00C_LIGHT_0045.fits
Saving fully-calibrated image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-39-27_20.00sec_-4.90C_LIGHT_0014.fits
Saving fully-calibrated image wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cam-08-Q2b1x1_224123_TTUQ2b1x1_24786_24KicoFY/wcs_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015.fits
Preparing the HTML report for the field Cam-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out129476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99814.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 28s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 20s
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Considering the candidate 176136_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176136_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:26:39.43 +59:31:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.912 462212427507909120 051.66428235620 +59.52669111788 13.5422 12.8341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176139_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176139_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:58:57.50 +61:57:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 4.771 474798674548914432 059.73817847173 +61.96514901471 13.9366 12.8963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176144_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176144_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:04:23.53 +65:46:44.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 176145_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176145_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:49:52.09 +59:17:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176148_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176148_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:53:01.39 +62:36:03.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 176152_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176152_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:29.39 +64:49:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176154_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176154_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:57:15.87 +59:56:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176155_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176155_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:19:33.57 +58:43:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176157_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176157_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:56:39.49 +60:24:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176161_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 176161_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:50:55.21 +61:54:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178157_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 178157_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:49.73 +59:55:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178273_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 178273_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:07:02.56 +58:35:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.541 460481693126283904 046.76002050074 +58.58781226595 10.2131 8.7212 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179154_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 179154_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:30:05.81 +58:50:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180879_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 180879_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:20:20.96 +65:39:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181095_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 181095_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:53:31.80 +63:22:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181658_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 181658_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:20:15.79 +65:40:11.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181766_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 181766_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:59:09.79 +58:01:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181968_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 181968_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:23:43.20 +58:42:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182186_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 182186_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:53:29.16 +64:41:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182481_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 182481_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:32.24 +63:12:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182909_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 182909_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:51:13.66 +60:26:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183137_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 183137_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:11:19.63 +57:56:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184052_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184052_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:26:37.06 +64:14:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184222_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184222_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:33:30.02 +57:52:22.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 184330_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184330_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:11:30.89 +57:52:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184368_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184368_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:54:49.64 +63:44:60.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184382_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184382_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:54.27 +59:56:56.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184471_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184471_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:10:56.51 +61:08:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184804_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184804_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 04:00:17.68 +57:57:33.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184820_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 184820_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:08:42.83 +62:22:20.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185098_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 185098_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:58:40.74 +57:49:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185159_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 185159_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:26:55.04 +60:23:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185283_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 185283_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:11:55.02 +64:21:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185874_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 185874_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:23:36.06 +62:22:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186128_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 186128_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:17:52.69 +58:47:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186456_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 186456_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:33:32.07 +59:26:03.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186639_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 186639_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:54:10.96 +58:39:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186645_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 186645_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:23:20.84 +58:44:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186668_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 186668_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:28:28.01 +59:55:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187164_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 187164_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:34:45.15 +63:54:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187284_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 187284_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:56:47.86 +58:29:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187457_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 187457_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:36:23.26 +61:36:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187616_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 187616_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:23:36.30 +58:59:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187984_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 187984_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:20:59.75 +60:00:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188109_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 188109_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:50:45.19 +59:14:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.268 473319693972169216 057.68706139096 +59.24949278983 13.8189 12.7588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188606_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 188606_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:53:19.76 +60:18:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189002_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 189002_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:53:59.08 +62:04:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.709 474914535587508864 058.49519205117 +62.08051969166 13.5655 12.4973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189240_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 189240_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:29.38 +59:56:55.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189465_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 189465_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:37:45.20 +59:32:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189504_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 189504_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:44:48.92 +62:16:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.401 486646359015166336 056.20380491004 +62.26866627939 13.9269 12.9766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190192_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 190192_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:19:07.65 +57:52:12.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190619_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 190619_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:56:13.15 +65:06:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191644_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 191644_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:20:06.66 +62:31:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194043_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 194043_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:38:56.95 +65:16:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21396_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 21396_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84933_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 84933_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:55:57.99 +61:31:18.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64776_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 64776_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:49.31 +60:54:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124836_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 124836_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67405_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 67405_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:40:40.28 +61:05:05.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19478_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 19478_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:09:37.75 +57:43:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103058_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 103058_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99814_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 99814_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165618_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 165618_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:59:15.73 +60:18:03.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32499_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 32499_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55998_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 55998_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:54:19.73 +59:29:18.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82599_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 82599_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43428_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 43428_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21101_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 21101_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128848_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 128848_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35447_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 35447_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18016_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 18016_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:59:15.99 +58:13:22.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46728_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 46728_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136288_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 136288_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35348_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 35348_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125559_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 125559_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71412_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 71412_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14217_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 14217_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:42:07.39 +57:52:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58893_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 58893_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32033_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 32033_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27443_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 27443_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139457_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 139457_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80737_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 80737_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148915_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 148915_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86913_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 86913_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:23:07.03 +62:07:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138406_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 138406_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 04:03:11.44 +64:13:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55891_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 55891_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135901_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 135901_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:37:09.51 +64:20:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30952_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 30952_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29507_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 29507_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25636_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 25636_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77632_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 77632_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94972_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 94972_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:04:49.03 +62:24:24.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91149_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 91149_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:14:27.31 +62:13:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27289_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 27289_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:55:04.41 +57:50:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53583_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 53583_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15970_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 15970_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81820_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 81820_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119927_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 119927_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79424_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 79424_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78907_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 78907_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:05:09.28 +61:14:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17182_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 17182_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138021_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 138021_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:56:47.80 +63:27:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42436_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 42436_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:08:10.83 +59:02:12.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25210_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 25210_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135975_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 135975_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129882_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 129882_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:11:44.84 +64:24:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130983_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 130983_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166647_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 166647_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:48:03.49 +62:16:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43427_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 43427_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130384_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 130384_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118847_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 118847_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95267_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 95267_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:01:07.48 +62:11:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96818_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 96818_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:03:13.28 +62:20:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112091_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 112091_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129476_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 129476_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 03:14:02.56 +64:29:01.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88941_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 88941_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61816_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 61816_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63368_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 63368_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55905_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
The candidate 55905_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015 did not pass the final checks
**** FOUND 02:52:04.29 +59:25:17.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101711_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 101711_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56483_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
Preparing report for the candidate 56483_fd_Cam-08-Q2b1x1_2026-04-09_22-40-19_20.00sec_-5.00C_LIGHT_0015
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 51s
Prepared the HTML report for the field Cam-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:08:10.83 +59:02:12.7
02:54:19.68 +59:29:18.4
03:04:48.93 +62:24:24.5
02:59:40.14 +62:33:39.3
03:05:29.70 +62:47:01.2
02:45:05.62 +65:01:20.9
03:00:48.04 +65:01:10.1
02:56:24.52 +64:50:29.8
02:48:50.66 +64:11:50.7
03:16:46.71 +64:45:03.7
03:30:08.95 +64:46:31.0
02:48:00.11 +63:45:44.1
02:46:27.57 +63:40:33.0
02:51:21.12 +63:25:28.2
03:04:57.04 +63:47:36.2
03:58:40.88 +64:09:34.7
03:21:27.62 +63:15:36.2
03:35:40.28 +57:55:52.4
03:24:15.13 +57:51:08.9
03:08:46.31 +57:48:41.8
02:57:11.63 +57:30:30.7
02:59:06.30 +57:48:33.6
03:12:53.33 +58:12:05.1
03:00:52.89 +58:01:54.6
03:11:00.32 +58:25:10.7
03:19:13.93 +58:42:01.7
02:57:39.75 +58:12:52.9
02:56:49.69 +58:14:29.2
02:55:32.12 +58:16:20.3
04:02:29.84 +59:19:24.0
03:00:51.06 +58:56:33.3
03:38:09.74 +59:40:45.3
02:53:45.32 +58:57:49.4
03:24:08.24 +60:05:54.4
03:00:45.53 +59:43:07.3
02:51:46.70 +59:27:47.0
03:54:25.44 +60:39:20.4
03:03:27.68 +60:07:46.4
03:06:39.86 +60:18:08.9
03:10:30.40 +60:53:32.8
03:26:33.04 +61:33:44.2
03:18:04.67 +61:34:07.0
02:50:12.71 +60:56:24.0
03:04:22.09 +61:25:44.0
03:41:00.48 +62:02:21.6
02:58:15.24 +61:43:08.2
02:58:19.49 +62:25:47.0
########### Completed Cam-08-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
03:04:48.93 +62:24:24.5
03:08:10.83 +59:02:12.7
02:54:19.68 +59:29:18.4
02:57:11.63 +57:30:30.7
02:48:50.66 +64:11:50.7
03:05:29.70 +62:47:01.2
02:58:19.49 +62:25:47.0
02:56:49.69 +58:14:29.2
03:41:00.48 +62:02:21.6
03:38:09.74 +59:40:45.3
03:08:46.31 +57:48:41.8
03:30:08.95 +64:46:31.0
04:02:29.84 +59:19:24.0
02:53:45.32 +58:57:49.4
03:04:57.04 +63:47:36.2
02:55:32.12 +58:16:20.3
03:16:46.71 +64:45:03.7
03:10:30.40 +60:53:32.8
03:54:25.44 +60:39:20.4
02:57:39.75 +58:12:52.9
03:00:52.89 +58:01:54.6
03:58:40.88 +64:09:34.7
02:50:12.71 +60:56:24.0
03:21:27.62 +63:15:36.2
03:00:45.53 +59:43:07.3
03:19:13.93 +58:42:01.7
03:11:00.32 +58:25:10.7
03:12:53.33 +58:12:05.1
03:26:33.04 +61:33:44.2
03:24:08.24 +60:05:54.4
03:35:40.28 +57:55:52.4
03:04:22.09 +61:25:44.0
02:56:24.52 +64:50:29.8
03:18:04.67 +61:34:07.0
03:24:15.13 +57:51:08.9
02:59:06.30 +57:48:33.6
02:51:21.12 +63:25:28.2
02:46:27.57 +63:40:33.0
03:00:51.06 +58:56:33.3
02:48:00.11 +63:45:44.1
03:00:48.04 +65:01:10.1
02:45:05.62 +65:01:20.9
02:58:15.24 +61:43:08.2
03:03:27.68 +60:07:46.4
03:06:39.86 +60:18:08.9
02:59:40.14 +62:33:39.3
02:51:46.70 +59:27:47.0
###################################################################################
03:04:48.93 +62:24:24.5 -- not an asteroid (will add it to exclusion list)
03:08:10.83 +59:02:12.7 -- not an asteroid (will add it to exclusion list)
02:54:19.68 +59:29:18.4 -- not an asteroid (will add it to exclusion list)
02:57:11.63 +57:30:30.7 -- not an asteroid (will add it to exclusion list)
02:48:50.66 +64:11:50.7 -- not an asteroid (will add it to exclusion list)
03:05:29.70 +62:47:01.2 -- not an asteroid (will add it to exclusion list)
02:58:19.49 +62:25:47.0 -- not an asteroid (will add it to exclusion list)
02:56:49.69 +58:14:29.2 -- not an asteroid (will add it to exclusion list)
03:41:00.48 +62:02:21.6 -- not an asteroid (will add it to exclusion list)
03:38:09.74 +59:40:45.3 -- not an asteroid (will add it to exclusion list)
03:08:46.31 +57:48:41.8 -- not an asteroid (will add it to exclusion list)
03:30:08.95 +64:46:31.0 -- not an asteroid (will add it to exclusion list)
04:02:29.84 +59:19:24.0 -- not an asteroid (will add it to exclusion list)
02:53:45.32 +58:57:49.4 -- not an asteroid (will add it to exclusion list)
03:04:57.04 +63:47:36.2 -- not an asteroid (will add it to exclusion list)
02:55:32.12 +58:16:20.3 -- not an asteroid (will add it to exclusion list)
03:16:46.71 +64:45:03.7 -- not an asteroid (will add it to exclusion list)
03:10:30.40 +60:53:32.8 -- not an asteroid (will add it to exclusion list)
03:54:25.44 +60:39:20.4 -- not an asteroid (will add it to exclusion list)
02:57:39.75 +58:12:52.9 -- not an asteroid (will add it to exclusion list)
03:00:52.89 +58:01:54.6 -- not an asteroid (will add it to exclusion list)
03:58:40.88 +64:09:34.7 -- not an asteroid (will add it to exclusion list)
02:50:12.71 +60:56:24.0 -- not an asteroid (will add it to exclusion list)
03:21:27.62 +63:15:36.2 -- not an asteroid (will add it to exclusion list)
03:00:45.53 +59:43:07.3 -- not an asteroid (will add it to exclusion list)
03:19:13.93 +58:42:01.7 -- not an asteroid (will add it to exclusion list)
03:11:00.32 +58:25:10.7 -- not an asteroid (will add it to exclusion list)
03:12:53.33 +58:12:05.1 -- not an asteroid (will add it to exclusion list)
03:26:33.04 +61:33:44.2 -- not an asteroid (will add it to exclusion list)
03:24:08.24 +60:05:54.4 -- not an asteroid (will add it to exclusion list)
03:35:40.28 +57:55:52.4 -- not an asteroid (will add it to exclusion list)
03:04:22.09 +61:25:44.0 -- not an asteroid (will add it to exclusion list)
02:56:24.52 +64:50:29.8 -- not an asteroid (will add it to exclusion list)
03:18:04.67 +61:34:07.0 -- not an asteroid (will add it to exclusion list)
03:24:15.13 +57:51:08.9 -- not an asteroid (will add it to exclusion list)
02:59:06.30 +57:48:33.6 -- not an asteroid (will add it to exclusion list)
02:51:21.12 +63:25:28.2 -- not an asteroid (will add it to exclusion list)
02:46:27.57 +63:40:33.0 -- not an asteroid (will add it to exclusion list)
03:00:51.06 +58:56:33.3 -- not an asteroid (will add it to exclusion list)
02:48:00.11 +63:45:44.1 -- not an asteroid (will add it to exclusion list)
03:00:48.04 +65:01:10.1 -- not an asteroid (will add it to exclusion list)
02:45:05.62 +65:01:20.9 -- not an asteroid (will add it to exclusion list)
02:58:15.24 +61:43:08.2 -- not an asteroid (will add it to exclusion list)
03:03:27.68 +60:07:46.4 -- not an asteroid (will add it to exclusion list)
03:06:39.86 +60:18:08.9 -- not an asteroid (will add it to exclusion list)
02:59:40.14 +62:33:39.3 -- not an asteroid (will add it to exclusion list)
02:51:46.70 +59:27:47.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
02:45:05.62 +65:01:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:46:27.57 +63:40:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:00.11 +63:45:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:50.66 +64:11:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:12.71 +60:56:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:21.12 +63:25:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:51:46.70 +59:27:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:53:45.32 +58:57:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:19.68 +59:29:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:32.12 +58:16:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:24.52 +64:50:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:49.69 +58:14:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:11.63 +57:30:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:39.75 +58:12:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:15.24 +61:43:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:19.49 +62:25:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:06.30 +57:48:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:40.14 +62:33:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:45.53 +59:43:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:48.04 +65:01:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:51.06 +58:56:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:52.89 +58:01:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:27.68 +60:07:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:22.09 +61:25:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:48.93 +62:24:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:57.04 +63:47:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:29.70 +62:47:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:06:39.86 +60:18:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:10.83 +59:02:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:46.31 +57:48:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:10:30.40 +60:53:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:00.32 +58:25:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:53.33 +58:12:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:46.71 +64:45:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:04.67 +61:34:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:13.93 +58:42:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:27.62 +63:15:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:08.24 +60:05:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:15.13 +57:51:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:26:33.04 +61:33:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:08.95 +64:46:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:40.28 +57:55:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:09.74 +59:40:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:00.48 +62:02:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:25.44 +60:39:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:40.88 +64:09:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:29.84 +59:19:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
02:45:05.62 +65:01:20.9 -- a known variable star
02:46:27.57 +63:40:33.0 -- a known variable star
02:48:00.11 +63:45:44.1 -- a known variable star
02:48:50.66 +64:11:50.7 -- a known variable star
02:50:12.71 +60:56:24.0 -- not a known variable star
02:51:21.12 +63:25:28.2 -- a known variable star
02:51:46.70 +59:27:47.0 -- a known variable star
02:53:45.32 +58:57:49.4 -- a known variable star
02:54:19.68 +59:29:18.4 -- a known variable star
02:55:32.12 +58:16:20.3 -- a known variable star
02:56:24.52 +64:50:29.8 -- a known variable star
02:56:49.69 +58:14:29.2 -- not a known variable star
02:57:11.63 +57:30:30.7 -- a known variable star
02:57:39.75 +58:12:52.9 -- a known variable star
02:58:15.24 +61:43:08.2 -- a known variable star
02:58:19.49 +62:25:47.0 -- a known variable star
02:59:06.30 +57:48:33.6 -- a known variable star
02:59:40.14 +62:33:39.3 -- not a known variable star
03:00:45.53 +59:43:07.3 -- a known variable star
03:00:48.04 +65:01:10.1 -- a known variable star
03:00:51.06 +58:56:33.3 -- a known variable star
03:00:52.89 +58:01:54.6 -- not a known variable star
03:03:27.68 +60:07:46.4 -- a known variable star
03:04:22.09 +61:25:44.0 -- a known variable star
03:04:48.93 +62:24:24.5 -- a known variable star
03:04:57.04 +63:47:36.2 -- a known variable star
03:05:29.70 +62:47:01.2 -- a known variable star
03:06:39.86 +60:18:08.9 -- not a known variable star
03:08:10.83 +59:02:12.7 -- not a known variable star
03:08:46.31 +57:48:41.8 -- not a known variable star
03:10:30.40 +60:53:32.8 -- a known variable star
03:11:00.32 +58:25:10.7 -- a known variable star
03:12:53.33 +58:12:05.1 -- a known variable star
03:16:46.71 +64:45:03.7 -- a known variable star
03:18:04.67 +61:34:07.0 -- a known variable star
03:19:13.93 +58:42:01.7 -- a known variable star
03:21:27.62 +63:15:36.2 -- a known variable star
03:24:08.24 +60:05:54.4 -- a known variable star
03:24:15.13 +57:51:08.9 -- a known variable star
03:26:33.04 +61:33:44.2 -- a known variable star
03:30:08.95 +64:46:31.0 -- a known variable star
03:35:40.28 +57:55:52.4 -- a known variable star
03:38:09.74 +59:40:45.3 -- a known variable star
03:41:00.48 +62:02:21.6 -- a known variable star
03:54:25.44 +60:39:20.4 -- a known variable star
03:58:40.88 +64:09:34.7 -- a known variable star
04:02:29.84 +59:19:24.0 -- a known variable star
Found 7 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
47 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
02:45:05.62 +65:01:20.9
02:46:27.57 +63:40:33.0
02:48:00.11 +63:45:44.1
02:48:50.66 +64:11:50.7
02:50:12.71 +60:56:24.0
02:51:21.12 +63:25:28.2
02:51:46.70 +59:27:47.0
02:53:45.32 +58:57:49.4
02:54:19.68 +59:29:18.4
02:55:32.12 +58:16:20.3
02:56:24.52 +64:50:29.8
02:56:49.69 +58:14:29.2
02:57:11.63 +57:30:30.7
02:57:39.75 +58:12:52.9
02:58:15.24 +61:43:08.2
02:58:19.49 +62:25:47.0
02:59:06.30 +57:48:33.6
02:59:40.14 +62:33:39.3
03:00:45.53 +59:43:07.3
03:00:48.04 +65:01:10.1
03:00:51.06 +58:56:33.3
03:00:52.89 +58:01:54.6
03:03:27.68 +60:07:46.4
03:04:22.09 +61:25:44.0
03:04:48.93 +62:24:24.5
03:04:57.04 +63:47:36.2
03:05:29.70 +62:47:01.2
03:06:39.86 +60:18:08.9
03:08:10.83 +59:02:12.7
03:08:46.31 +57:48:41.8
03:10:30.40 +60:53:32.8
03:11:00.32 +58:25:10.7
03:12:53.33 +58:12:05.1
03:16:46.71 +64:45:03.7
03:18:04.67 +61:34:07.0
03:19:13.93 +58:42:01.7
03:21:27.62 +63:15:36.2
03:24:08.24 +60:05:54.4
03:24:15.13 +57:51:08.9
03:26:33.04 +61:33:44.2
03:30:08.95 +64:46:31.0
03:35:40.28 +57:55:52.4
03:38:09.74 +59:40:45.3
03:41:00.48 +62:02:21.6
03:54:25.44 +60:39:20.4
03:58:40.88 +64:09:34.7
04:02:29.84 +59:19:24.0
02:48:50.56 +64:11:51.3
03:14:02.56 +64:29:01.8
02:59:15.73 +60:18:03.2
03:26:39.43 +59:31:37.0
03:58:57.50 +61:57:50.4
03:04:23.53 +65:46:44.2
02:53:01.39 +62:36:03.9
03:07:02.56 +58:35:20.5
03:50:45.19 +59:14:58.3
03:53:59.08 +62:04:49.4
03:44:48.92 +62:16:06.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461140.65251181 -observatory V36
23:38:03.78 -04:55:41.6 Mercury (0.2mag)
02:40:20.28 +15:32:38.6 Venus (-3.9mag)
00:01:12.40 -00:58:02.0 Mars (1.2mag)
07:10:09.51 +22:50:12.2 Jupiter (-2.1mag)
00:26:33.40 +00:32:32.9 Saturn (0.9mag)
03:46:29.80 +19:43:36.6 Uranus (5.8mag)
00:10:03.91 -00:20:16.2 Neptune (7.8mag)
20:33:28.01 -22:52:27.0 Pluto (14.5mag)
19:28:17.95 -26:02:00.2 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Apr 9 22:43 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461140.65251181:
07:10:02.96 +22:50:23.6 Io (5.7mag)
07:10:17.84 +22:49:52.4 Europa (5.9mag)
07:10:08.59 +22:50:06.4 Ganymede (5.3mag)
07:09:47.65 +22:51:02.8 Callisto (6.6mag)
07:13:44.13 +22:40:39.7 Himalia (15.3mag)
07:10:05.45 +22:50:20.5 Thebe (16.2mag)
07:13:47.57 +23:10:11.3 Elara (17.3mag)
07:08:38.50 +23:33:16.1 Pasiphae (17.4mag)
07:18:36.68 +22:47:36.6 Carme (18.5mag)
00:26:43.22 +00:32:23.6 Titan (8.8mag)
00:26:32.39 +00:32:49.0 Rhea (10.1mag)
00:26:25.00 +00:33:36.1 Iapetus (11.5mag)
00:26:46.88 +00:32:21.5 Hyperion (14.8mag)
00:28:14.78 +00:41:58.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 22:43 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.65251181:
15:09:55.91 -11:47:09.2 JWST
19:12:08.05 +14:50:50.5 Chandra
07:54:48.81 -35:34:36.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 22:43 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.65251181 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:18.80 -28:26:49.1 13.9mag P/2010 H2 (Vales)
05:02:40.04 -69:56:46.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:15.82 +31:23:58.0 17.2mag C/2017 K2 (PANSTARRS)
17:30:51.37 +09:50:57.1 17.6mag C/2021 G2 (ATLAS)
23:08:34.66 +29:00:22.2 17.0mag C/2022 E2 (ATLAS)
04:22:28.96 +25:52:37.1 15.9mag C/2022 N2 (PANSTARRS)
09:02:21.06 +31:57:55.7 16.2mag C/2022 QE78 (ATLAS)
08:30:18.99 -00:47:10.8 17.3mag C/2022 R6 (PANSTARRS)
18:54:57.59 +18:02:10.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:27.42 -11:36:21.5 17.5mag P/2023 B1 (PANSTARRS)
09:10:33.89 -12:50:12.8 17.6mag C/2023 F3 (ATLAS)
21:48:02.42 +62:34:36.4 17.5mag C/2023 H5 (Lemmon)
19:23:48.95 -03:38:58.6 14.2mag C/2023 R1 (PANSTARRS)
21:40:35.35 +85:07:07.5 17.8mag C/2023 X2 (Lemmon)
06:15:34.29 +63:32:54.6 17.1mag C/2024 A1 (ATLAS)
05:00:21.24 +16:12:13.8 10.7mag C/2024 E1 (Wierzchos)
16:22:52.66 +05:25:46.4 17.4mag C/2024 G6 (ATLAS)
20:18:59.78 +13:42:37.9 14.7mag C/2024 J3 (ATLAS)
03:21:11.04 -23:17:26.5 16.4mag C/2024 T5 (ATLAS)
05:11:51.04 +46:46:43.2 17.7mag C/2025 J1 (Borisov)
14:03:05.82 +41:05:52.6 14.9mag C/2025 L1 (ATLAS)
03:16:13.96 -25:19:22.0 17.8mag C/2025 Q3 (ATLAS)
23:06:39.48 +19:42:44.1 9.4mag C/2025 R3 (PANSTARRS)
12:56:39.89 +02:38:55.1 17.5mag C/2025 Y1 (ATLAS)
02:29:44.69 +03:30:26.8 10.9mag C/2026 A1 (MAPS)
23:42:40.37 +36:05:14.1 14.4mag C/2026 B2 (Sun-Gao)
18:31:32.01 -10:01:28.8 12.2mag 10P/Tempel
15:08:02.54 +03:46:39.8 13.5mag 24P/Schaumasse
11:04:29.13 -01:43:20.2 15.7mag 29P/Schwassmann-Wachmann
17:58:48.68 -09:50:00.4 17.8mag 40P/Vaisala
10:38:06.85 -04:35:16.3 16.8mag 43P/Wolf-Harrington
01:39:38.41 +16:29:03.8 17.2mag 47P/Ashbrook-Jackson
07:00:11.16 +38:15:21.6 17.0mag 63P/Wild
23:21:31.11 -12:09:43.6 15.7mag 65P/Gunn
03:47:50.07 +19:11:45.2 15.9mag 76P/West-Kohoutek-Ikemura
00:52:42.44 +07:04:25.6 14.4mag 78P/Gehrels
22:45:02.60 -11:06:56.7 14.6mag 88P/Howell
01:54:01.48 +19:03:21.0 15.1mag 93P/Lovas
04:43:58.78 +31:57:48.6 16.3mag 123P/West-Hartley
08:21:50.16 +41:03:41.9 16.2mag 124P/Mrkos
02:24:13.75 +13:42:40.7 16.4mag 128P/Shoemaker-Holt
02:36:05.81 +13:45:55.6 17.5mag 131P/Mueller
00:55:50.10 +11:07:53.0 10.9mag 141P/Machholz
01:05:28.64 +02:40:36.5 11.0mag 141P-A/Machholz
23:53:46.90 -01:09:42.9 13.5mag 141P-D/Machholz
01:35:11.16 +04:23:50.3 17.9mag 141P-I/Machholz
00:46:06.49 -04:27:19.5 15.2mag 162P/SidingSpring
10:29:51.60 +31:15:13.5 17.9mag 164P/Christensen
06:25:42.06 +24:25:21.1 17.9mag 198P/ODAS
15:01:48.52 -00:42:43.5 17.5mag 210P/Christensen
21:21:24.90 -12:51:45.9 17.5mag 218P/LINEAR
17:14:35.72 -14:37:27.0 16.2mag 235P/LINEAR
05:21:57.97 +34:13:22.0 16.7mag 240P/NEAT
07:35:47.55 -05:49:11.1 17.7mag 242P/Spahr
15:44:45.11 +06:35:33.3 17.5mag 391P/Kowalski
07:32:06.64 +21:20:24.0 17.6mag 450P/LONEOS
05:27:27.17 +45:22:34.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 22:43 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 9 22:43 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:18:48.927 -23:32:12.08 AT 2026ike 2026-02-12.51 20.2
08:47:41.490 -21:46:40.10 AT 2026ikd 2026-03-28.41 19.49
08:34:30.248 -07:09:24.85 AT 2026ikc 2026-03-29.44 19.28
13:21:25.078 +79:09:18.53 AT 2026ikb 2026-03-25.43 20.7322
09:05:18.124 -19:48:21.41 AT 2026ika 2026-03-09.36 20.58
08:38:25.468 +06:11:03.79 AT 2026ijz 2026-03-09.32 21.99
08:00:34.010 +04:48:18.04 AT 2026ijy 2026-03-09.31 21.07
09:02:07.082 +07:27:03.87 AT 2026ijx 2026-02-17.43 21.29
10:37:20.784 +30:59:50.95 AT 2026ijw 2026-03-10.33 20.2
16:00:37.915 +06:38:30.61 AT 2026ijv 2026-03-28.57 20.5
13:51:30.137 +25:53:04.17 AT 2026iju 2026-03-28.41 20.07
12:52:01.341 -19:06:48.80 AT 2026ijt 2026-01-28.59 20.22
11:38:25.995 -11:34:40.48 AT 2026ijs 2026-01-16.56 21.1
07:12:41.661 +56:25:20.59 AT 2026ijr 2026-01-19.40 20.76
09:34:48.813 +06:57:40.76 AT 2026ijq 2026-01-26.43 21.57
10:49:59.384 +25:17:19.22 AT 2026ijp 2026-04-04.17 19.836
08:20:22.449 +03:44:22.06 AT 2026ijo 2026-04-02.18 19.8276
06:41:34.987 -19:08:36.17 AT 2026ijn 2026-02-05.26 20.38
12:35:13.975 +41:45:24.96 AT 2026ijm 2026-04-02.31 19.9925
13:25:11.624 +08:21:44.99 AT 2026ijl 2026-03-27.40 20.8103
-rw-r--r-- 1 apache apache 30K Apr 9 22:43 tns_transients_list.txt
